Observations were conducted as part of the Thousand Pulsar Array (TPA) program, itself part of the larger MeerTime project on the MeerKAT telescope. Details of the project as a whole and the observational setup can be found in [1]} and [2]}. In brief, we used the observational band from 896 to 1671 MHz with 928 frequency channels. The data are folded into sub-integrations each of length 8 s for the duration of the observation and there are 1024 phase bins per pulse period. Polarization calibration is carried out using the procedures described in detail in [3]}. Flux calibration is carried out as described in [4]}. All these operations are performed by the processing pipeline meerpipehttps://github.com/aparthas3112/meerpipe which produces RFI-excised, polarization- and flux-calibrated output products in psrfits format [5]}. A more complete description of the pipeline is reported in [6]}. In this paper we use the same data set described in detail in [4]}.
